How Many Templates for GW Chirp Detection? The Minimal-Match Issue Revisited

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

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submitted to Class. Quantum Grav. Typing error in eq. (4.8) fixed; figure replaced in version 2

Scientific paper

10.1088/0264-9381/21/21/013

In a recent paper dealing with maximum likelihood detection of gravitational wave chirps from coalescing binaries with unknown parameters we introduced an accurate representation of the no-signal cumulative distribution of the supremum of the whole correlator bank. This result can be used to derive a refined estimate of the number of templates yielding the best tradeoff between detector's performance (in terms of lost signals among those potentially detectable) and computational burden.

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